Fig. 5.

Observed rotational splittings (open symbols) for modes of degrees l = 1 (circles) and l = 2 (squares) plotted as a function of the parameter ζ obtained from the best-fit stellar models (ζ measures the trapping of the modes, with ζ → 0 for p-dominated and ζ → 1 for g-dominated modes). The splittings obtained with the inverted values of ⟨Ω⟩g and ⟨Ω⟩p (see Sect. 4) are shown as filled symbols. The dashed and dotted lines show the expected rotational splittings for l = 1 and 2 modes, respectively, when fitting Eq. (8) to the observations.
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